TY - JOUR
T1 - The Atacama Cosmology Telescope
T2 - High-resolution Sunyaev-Zel'dovich Array observations of ACT SZE-Selected clusters from the equatorial strip
AU - Reese, Erik D.
AU - Mroczkowski, Tony
AU - Menanteau, Felipe
AU - Hilton, Matt
AU - Sievers, Jonathan
AU - Aguirre, Paula
AU - Appel, John William
AU - Baker, Andrew J.
AU - Bond, J. Richard
AU - Das, Sudeep
AU - Devlin, Mark J.
AU - Dicker, Simon R.
AU - Dünner, Rolando
AU - Essinger-Hileman, Thomas
AU - Fowler, Joseph W.
AU - Hajian, Amir
AU - Halpern, Mark
AU - Hasselfield, Matthew
AU - Hill, J. Colin
AU - Hincks, Adam D.
AU - Huffenberger, Kevin M.
AU - Hughes, John P.
AU - Irwin, Kent D.
AU - Klein, Jeff
AU - Kosowsky, Arthur
AU - Lin, Yen Ting
AU - Marriage, Tobias A.
AU - Marsden, Danica
AU - Moodley, Kavilan
AU - Niemack, Michael D.
AU - Nolta, Michael R.
AU - Page, Lyman A.
AU - Parker, Lucas
AU - Partridge, Bruce
AU - Rojas, Felipe
AU - Sehgal, Neelima
AU - Sifón, Cristóbal
AU - Spergel, David N.
AU - Staggs, Suzanne T.
AU - Swetz, Daniel S.
AU - Switzer, Eric R.
AU - Thornton, Robert
AU - Trac, Hy
AU - Wollack, Edward J.
PY - 2012/5/20
Y1 - 2012/5/20
N2 - We present follow-up observations with the Sunyaev-Zel'dovich Array (SZA) of optically confirmed galaxy clusters found in the equatorial survey region of the Atacama Cosmology Telescope (ACT): ACT-CL J0022-0036, ACT-CL J2051+0057, and ACT-CL J2337+0016. ACT-CL J0022-0036 is a newly discovered, massive (≃ 1015 M), high-redshift (z = 0.81) cluster revealed by ACT through the Sunyaev-Zel'dovich effect (SZE). Deep, targeted observations with the SZA allow us to probe a broader range of cluster spatial scales, better disentangle cluster decrements from radio point-source emission, and derive more robust integrated SZE flux and mass estimates than we can with ACT data alone. For the two clusters we detect with the SZA we compute integrated SZE signal and derive masses from the SZA data only. ACT-CL J2337+0016, also known as A2631, has archival Chandra data that allow an additional X-ray-based mass estimate. Optical richness is also used to estimate cluster masses and shows good agreement with the SZE and X-ray-based estimates. Based on the point sources detected by the SZA in these three cluster fields and an extrapolation to ACT's frequency, we estimate that point sources could be contaminating the SZE decrement at the ≲ 20% level for some fraction of clusters.
AB - We present follow-up observations with the Sunyaev-Zel'dovich Array (SZA) of optically confirmed galaxy clusters found in the equatorial survey region of the Atacama Cosmology Telescope (ACT): ACT-CL J0022-0036, ACT-CL J2051+0057, and ACT-CL J2337+0016. ACT-CL J0022-0036 is a newly discovered, massive (≃ 1015 M), high-redshift (z = 0.81) cluster revealed by ACT through the Sunyaev-Zel'dovich effect (SZE). Deep, targeted observations with the SZA allow us to probe a broader range of cluster spatial scales, better disentangle cluster decrements from radio point-source emission, and derive more robust integrated SZE flux and mass estimates than we can with ACT data alone. For the two clusters we detect with the SZA we compute integrated SZE signal and derive masses from the SZA data only. ACT-CL J2337+0016, also known as A2631, has archival Chandra data that allow an additional X-ray-based mass estimate. Optical richness is also used to estimate cluster masses and shows good agreement with the SZE and X-ray-based estimates. Based on the point sources detected by the SZA in these three cluster fields and an extrapolation to ACT's frequency, we estimate that point sources could be contaminating the SZE decrement at the ≲ 20% level for some fraction of clusters.
KW - cosmic background radiation
KW - cosmology: observations
KW - galaxies: clusters: general
KW - techniques: interferometric
KW - X-rays: galaxies: clusters
UR - https://www.scopus.com/pages/publications/84860733273
U2 - 10.1088/0004-637X/751/1/12
DO - 10.1088/0004-637X/751/1/12
M3 - Article
AN - SCOPUS:84860733273
SN - 0004-637X
VL - 751
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 1
M1 - 12
ER -